SDO HMI 2011-04-30 22:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.86 | 186.22 | 42.79 | 366.70 | 20.42 | 186.62 | 72.37 | 292.50 | 0.9656 | 152.1 | 15.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.05 | 36.82 | 6.34 | 111.28 | 20.09 | 192.92 | 78.66 | 291.15 | 0.9880 | 288.5 | -58.7 | |
| 4.19 | -1.00 | 12.27 | -1.00 | 19.98 | 192.22 | 77.96 | 291.13 | 0.9862 | -366.5 | 999999 | |
| 0.00 | 1.34 | 0.00 | 2.80 | 19.61 | 188.18 | 73.92 | 291.36 | 0.9729 | -155.0 | -190.5 | |
| 0.00 | 3.03 | 0.00 | 5.77 | 19.75 | 186.55 | 72.29 | 291.78 | 0.9666 | -69.0 | -68.5 | |
| 0.00 | 0.89 | 0.00 | 1.68 | 19.97 | 186.37 | 72.11 | 292.03 | 0.9660 | -141.0 | -147.9 | |
| 0.00 | 4.81 | 0.00 | 9.31 | 20.35 | 186.71 | 72.45 | 292.36 | 0.9678 | -196.0 | -171.8 | |
| 1.16 | 130.15 | 2.05 | 220.10 | 20.28 | 185.27 | 71.02 | 292.54 | 0.9616 | 227.6 | 62.7 | |
| 1.25 | -7.00 | 2.12 | -7.00 | 20.51 | 184.34 | 70.08 | 292.95 | 0.9576 | -131.5 | 999999 | |
| 6.95 | -7.00 | 11.49 | -7.00 | 20.44 | 183.89 | 69.63 | 292.97 | 0.9554 | 463.1 | 999999 | |
| 0.00 | 1.60 | 0.00 | 2.86 | 22.19 | 184.84 | 70.58 | 294.58 | 0.9615 | -353.0 | -360.3 | |
| 4.19 | -7.00 | 6.69 | -7.00 | 20.78 | 183.13 | 68.87 | 293.47 | 0.9521 | 709.4 | 999999 | |
| 1.07 | 6.60 | 1.83 | 11.32 | 22.11 | 184.16 | 69.90 | 294.63 | 0.9584 | 185.0 | 123.8 | |
| 0.00 | 0.98 | 0.00 | 1.58 | 21.76 | 183.03 | 68.78 | 294.50 | 0.9527 | 409.0 | 372.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |